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Photoevaporation obfuscates the distinction between wind and viscous angular momentum transport in protoplanetary discs

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Estimation of stellar parameters and mass accretion rate of classical T Tauri stars from LAMOST DR6

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Inward and outward migration of massive planets: moving towards a stalling radius

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A numerical approach to model chemistry of complex organic molecules in a protoplanetary disk

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Dynamical mass measurements of two protoplanetary discs

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Hyperion: the origin of the stars. A far UV space telescope for high-resolution spectroscopy over wide fields

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C18O Emission as an Effective Measure of Gas Masses of Protoplanetary Disks

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Time-dependent, long-term hydrodynamic simulations of the inner protoplanetary disk

L. Gehrig, D. Steiner, E. I. Vorobyov and M. Güdel
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The Relation between the Mass Accretion Rate and the Disk Mass in Class I Protostars

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The growth and migration of massive planets under the influence of external photoevaporation

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Dispersal of protoplanetary discs: how stellar properties and the local environment determine the pathway of evolution

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Monthly Notices of the Royal Astronomical Society 514 (2) 2315 (2022)
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On the time evolution of the Md−M⋆ and Ṁ–M⋆ correlations for protoplanetary discs: the viscous time-scale increases with stellar mass

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Secular evolution of MHD wind-driven discs: analytical solutions in the expanded α-framework

Benoît Tabone, Giovanni P Rosotti, Alexander J Cridland, Philip J Armitage and Giuseppe Lodato
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MHD disc winds can reproduce fast disc dispersal and the correlation between accretion rate and disc mass in Lupus

B Tabone, G P Rosotti, G Lodato, P J Armitage, A J Cridland and E F van Dishoeck
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The protoplanetary disk population in the ρ-Ophiuchi region L1688 and the time evolution of Class II YSOs

L. Testi, A. Natta, C. F. Manara, et al.
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Modelling the secular evolution of protoplanetary disc dust sizes – a comparison between the viscous and magnetic wind case

Francesco Zagaria, Giovanni P Rosotti, Cathie J Clarke and Benoît Tabone
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Stellar multiplicity affects the correlation between protoplanetary disc masses and accretion rates: binaries explain high accretors in Upper Sco

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Monthly Notices of the Royal Astronomical Society 512 (3) 3538 (2022)
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If you like C/O variations, you should have put a ring on it

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An ALMA Survey of Protoplanetary Disks in Lynds 1641

Sierra L. Grant, Catherine C. Espaillat, John Wendeborn, John J. Tobin, Enrique Macías, Anneliese Rilinger, Álvaro Ribas, S. Thomas Megeath, William J. Fischer, Nuria Calvet and Kyoung Hee Kim
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CO isotopolog line fluxes of viscously evolving disks

L. Trapman, A. D. Bosman, G. Rosotti, M. R. Hogerheijde and E. F. van Dishoeck
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MRI-active inner regions of protoplanetary discs. I. A detailed model of disc structure

Marija R Jankovic, James E Owen, Subhanjoy Mohanty and Jonathan C Tan
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Planet formation in intermediate-separation binary systems

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Large gaps and high accretion rates in photoevaporative transition disks with a dead zone

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Measuring the ratio of the gas and dust emission radii of protoplanetary disks in the Lupus star-forming region

E. Sanchis, L. Testi, A. Natta, et al.
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A backward-spinning star with two coplanar planets

Maria Hjorth, Simon Albrecht, Teruyuki Hirano, et al.
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Molecules with ALMA at Planet-forming Scales (MAPS). V. CO Gas Distributions

Ke Zhang, Alice S. Booth, Charles J. Law, Arthur D. Bosman, Kamber R. Schwarz, Edwin A. Bergin, Karin I. Öberg, Sean M. Andrews, Viviana V. Guzmán, Catherine Walsh, Chunhua Qi, Merel L. R. van ’t Hoff, Feng Long, David J. Wilner, Jane Huang, Ian Czekala, John D. Ilee, Gianni Cataldi, Jennifer B. Bergner, Yuri Aikawa, Richard Teague, Jaehan Bae, Ryan A. Loomis, Jenny K. Calahan, Felipe Alarcón, et al.
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PENELLOPE: The ESO data legacy program to complement the Hubble UV Legacy Library of Young Stars (ULLYSES)

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Destruction of Refractory Carbon Grains Drives the Final Stage of Protoplanetary Disk Chemistry

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Dust-depleted Inner Disks in a Large Sample of Transition Disks through Long-baseline ALMA Observations

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